Prominence Spectroscopy

Prominence Spectroscopy is a specialized observational method in solar physics that analyzes the spectral emissions of solar prominences to determine their physical properties, such as temperature, density, and velocity, by applying high-resolution spectroscopic techniques to understand their dynamics and thermodynamic structure within the solar atmosphere.

152

Publications

5.4K

Citations

266

Authors

147

Institutions

Publications per year

2017–2026

21

Variants

Solar Prominence Spectroscopy

Authors

266

  1. PH
    P. Heinzel

    Czech Academy of Sciences, Astronomical Institute, Czechia

    20 publications · 1.1K citations

    17

    h-index

  2. SG
    S. Gunár

    Czech Academy of Sciences, Astronomical Institute, Czechia

    13 publications · 829 citations

    13

    h-index

  3. JC
    J. C. Vial

    Institut d'Astrophysique Spatiale, France

    15 publications · 887 citations

    13

    h-index

  4. BS
    B. Schmieder

    Observatoire de Paris, France

    12 publications · 768 citations

    12

    h-index

  5. DA
    D. A. Landman

    University of Hawaii System, United States

    9 publications · 167 citations

    9

    h-index

1–5 of 266

Venues

  1. The Astrophysical Journal

    ApJ · 52 publications · 1.7K citations

    28

    h-index

  2. Solar Physics

    36 publications · 1K citations

    18

    h-index

  3. Astronomy and Astrophysics

    26 publications · 822 citations

    17

    h-index

  4. 5

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 58 citations

    4

    h-index

1–5